IPDxIRR_2F (Ionospheric plasma densities)#
Abstract: Access to the derived plasma characteristics at 1Hz (level 2 product).
%load_ext watermark
%watermark -i -v -p viresclient,pandas,xarray,matplotlib
Python implementation: CPython
Python version : 3.11.6
IPython version : 8.18.0
viresclient: 0.15.2
pandas : 2.1.3
xarray : 2023.12.0
matplotlib : 3.8.2
from viresclient import SwarmRequest
import datetime as dt
import matplotlib.pyplot as plt
from matplotlib.dates import DateFormatter
request = SwarmRequest()
IPDxIRR_2F product information#
Derived plasma characteristics at 1Hz, for each Swarm spacecraft.
Documentation:
Check what “IPD” data variables are available#
request.available_collections("IPD", details=False)
{'IPD': ['SW_OPER_IPDAIRR_2F', 'SW_OPER_IPDBIRR_2F', 'SW_OPER_IPDCIRR_2F']}
request.available_measurements("IPD")
['Ne',
'Te',
'Background_Ne',
'Foreground_Ne',
'PCP_flag',
'Grad_Ne_at_100km',
'Grad_Ne_at_50km',
'Grad_Ne_at_20km',
'Grad_Ne_at_PCP_edge',
'ROD',
'RODI10s',
'RODI20s',
'delta_Ne10s',
'delta_Ne20s',
'delta_Ne40s',
'Num_GPS_satellites',
'mVTEC',
'mROT',
'mROTI10s',
'mROTI20s',
'IBI_flag',
'Ionosphere_region_flag',
'IPIR_index',
'Ne_quality_flag',
'TEC_STD']
Fetch three hours of IPD data#
request.set_collection("SW_OPER_IPDAIRR_2F")
request.set_products(measurements=request.available_measurements("IPD"))
data = request.get_between(dt.datetime(2014, 12, 21, 0), dt.datetime(2014, 12, 21, 3))
Load and plot using pandas/matplotlib#
df = data.as_dataframe()
df.head()
| ROD | Foreground_Ne | Ne | RODI10s | Te | Latitude | Ionosphere_region_flag | Grad_Ne_at_20km | Longitude | Grad_Ne_at_100km | ... | Background_Ne | Grad_Ne_at_50km | PCP_flag | Ne_quality_flag | Radius | Spacecraft | RODI20s | delta_Ne20s | TEC_STD | delta_Ne10s | |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Timestamp | |||||||||||||||||||||
| 2014-12-21 00:00:00.196999936 | 0.0 | 1305371.000 | 1255163.2 | 10238.517220 | 2212.278353 | -4.693533 | 0 | -1.047788 | -128.771412 | -0.084919 | ... | 1343599.375 | -0.403940 | 0 | 20000 | 6.840395e+06 | A | 7764.002532 | 10266.500 | 3.131451 | 67.875 |
| 2014-12-21 00:00:01.196999936 | 0.0 | 1292046.000 | 1250357.7 | 3263.138721 | 2165.194729 | -4.757416 | 0 | 0.338403 | -128.772618 | -0.144009 | ... | 1343599.375 | 0.144877 | 0 | 20000 | 6.840404e+06 | A | 7181.496228 | 2830.850 | 3.122494 | 12961.600 |
| 2014-12-21 00:00:02.196999936 | 0.0 | 1312436.750 | 1265851.3 | 3263.138721 | 1544.874194 | -4.821298 | 0 | 0.133643 | -128.773822 | -0.058276 | ... | 1343599.375 | -0.123734 | 0 | 20000 | 6.840413e+06 | A | 7181.496228 | 0.000 | 3.113830 | 0.000 |
| 2014-12-21 00:00:03.196999936 | 0.0 | 1312436.750 | 1312436.8 | 3263.138721 | 1228.501871 | -4.885179 | 0 | 1.443077 | -128.775026 | -0.144613 | ... | 1343599.375 | -0.131441 | 0 | 20000 | 6.840422e+06 | A | 7390.308480 | 2194.925 | 3.104259 | 12393.550 |
| 2014-12-21 00:00:04.196999936 | 0.0 | 1315059.375 | 1253999.0 | 3263.138721 | 2681.512355 | -4.949060 | 0 | -1.948789 | -128.776229 | -0.039358 | ... | 1343599.375 | -0.403369 | 0 | 20000 | 6.840430e+06 | A | 7554.331699 | 9491.525 | 3.097484 | 21700.700 |
5 rows × 29 columns
df.columns
Index(['ROD', 'Foreground_Ne', 'Ne', 'RODI10s', 'Te', 'Latitude',
'Ionosphere_region_flag', 'Grad_Ne_at_20km', 'Longitude',
'Grad_Ne_at_100km', 'mROT', 'delta_Ne40s', 'mVTEC', 'IPIR_index',
'mROTI20s', 'Grad_Ne_at_PCP_edge', 'Num_GPS_satellites', 'mROTI10s',
'IBI_flag', 'Background_Ne', 'Grad_Ne_at_50km', 'PCP_flag',
'Ne_quality_flag', 'Radius', 'Spacecraft', 'RODI20s', 'delta_Ne20s',
'TEC_STD', 'delta_Ne10s'],
dtype='object')
fig, axes = plt.subplots(nrows=7, ncols=1, figsize=(20, 18), sharex=True)
df.plot(ax=axes[0], y=["Background_Ne", "Foreground_Ne", "Ne"], alpha=0.8)
df.plot(ax=axes[1], y=["Grad_Ne_at_100km", "Grad_Ne_at_50km", "Grad_Ne_at_20km"])
df.plot(ax=axes[2], y=["RODI10s", "RODI20s"])
df.plot(ax=axes[3], y=["ROD"])
df.plot(ax=axes[4], y=["mROT"])
df.plot(ax=axes[5], y=["delta_Ne10s", "delta_Ne20s", "delta_Ne40s"])
df.plot(ax=axes[6], y=["mROTI20s", "mROTI10s"])
axes[0].set_ylabel("[cm$^{-3}$]")
axes[1].set_ylabel("[cm$^{-3}$m$^{-1}$]")
axes[2].set_ylabel("[cm$^{-3}$s$^{-1}$]")
axes[3].set_ylabel("[cm$^{-3}$m$^{-1}$]")
axes[4].set_ylabel("[TECU s$^{-1}$]")
axes[5].set_ylabel("[cm$^{-3}$m$^{-1}$]")
axes[6].set_ylabel("[TECU s$^{-1}$]")
axes[6].set_xlabel("Timestamp")
for ax in axes:
# Reformat time axis
# https://www.earthdatascience.org/courses/earth-analytics-python/use-time-series-data-in-python/customize-dates--matplotlib-plots-python/
ax.xaxis.set_major_formatter(DateFormatter("%Y-%m-%d\n%H:%M:%S"))
ax.legend(loc="upper right")
ax.grid()
fig.subplots_adjust(hspace=0)
Load as xarray#
ds = data.as_xarray()
ds
<xarray.Dataset>
Dimensions: (Timestamp: 10800)
Coordinates:
* Timestamp (Timestamp) datetime64[ns] 2014-12-21T00:00:00.19...
Data variables: (12/29)
Spacecraft (Timestamp) object 'A' 'A' 'A' 'A' ... 'A' 'A' 'A'
ROD (Timestamp) float64 0.0 0.0 ... 7.28e+03 7.28e+03
Foreground_Ne (Timestamp) float64 1.305e+06 ... 6.488e+05
Ne (Timestamp) float64 1.255e+06 1.25e+06 ... 6.468e+05
RODI10s (Timestamp) float64 1.024e+04 3.263e+03 ... 503.7
Te (Timestamp) float64 2.212e+03 ... 1.723e+03
... ...
Ne_quality_flag (Timestamp) int32 20000 20000 20000 ... 10000 10000
Radius (Timestamp) float64 6.84e+06 6.84e+06 ... 6.835e+06
RODI20s (Timestamp) float64 7.764e+03 7.181e+03 ... 907.9
delta_Ne20s (Timestamp) float64 1.027e+04 ... 1.702e+03
TEC_STD (Timestamp) float64 3.131 3.122 ... 2.866 2.891
delta_Ne10s (Timestamp) float64 67.88 1.296e+04 ... 1.702e+03
Attributes:
Sources: ['SW_OPER_IPDAIRR_2F_20141221T000000_20141221T235959_0302']
MagneticModels: []
AppliedFilters: []Alternative plot setup#
To plot the data from xarray, we need a different plotting setup. This does however give us more control over the plot. The units are extracted directly from the xarray object.
fig, axes = plt.subplots(nrows=7, ncols=1, figsize=(20, 18), sharex=True)
def subplot(ax=None, y=None, **kwargs):
"""Plot combination of variables onto a given axis"""
units = ds[y[0]].units
for var in y:
ax.plot(ds["Timestamp"], ds[var], label=var, **kwargs)
if units != ds[var].units:
raise ValueError(f"Units mismatch for {var}")
ax.set_ylabel(f"[{units}]")
# Reformat time axis
# https://www.earthdatascience.org/courses/earth-analytics-python/use-time-series-data-in-python/customize-dates--matplotlib-plots-python/
ax.xaxis.set_major_formatter(DateFormatter("%Y-%m-%d\n%H:%M:%S"))
ax.legend(loc="upper right")
ax.grid()
subplot(ax=axes[0], y=["Background_Ne", "Foreground_Ne", "Ne"])
subplot(ax=axes[1], y=["Grad_Ne_at_100km", "Grad_Ne_at_50km", "Grad_Ne_at_20km"])
subplot(ax=axes[2], y=["RODI10s", "RODI20s"])
subplot(ax=axes[3], y=["ROD"])
subplot(ax=axes[4], y=["mROT"])
subplot(ax=axes[5], y=["delta_Ne10s", "delta_Ne20s", "delta_Ne40s"])
subplot(ax=axes[6], y=["mROTI20s", "mROTI10s"])
fig.subplots_adjust(hspace=0)